2019MNRAS.489.1304B


Query : 2019MNRAS.489.1304B

2019MNRAS.489.1304B - Mon. Not. R. Astron. Soc., 489, 1304-1320 (2019/October-2)

New β Cep pulsators discovered with K2 space photometry.

BURSSENS S., BOWMAN D.M., AERTS C., PEDERSEN M.G., MORAVVEJI E. and BUYSSCHAERT B.

Abstract (from CDS):

We present the discovery of three new β Cep pulsators, three new pulsators with frequency groupings, and frequency patterns in a B3Ib star, all of which show pulsations with frequencies as high as about 17 d–1, with K2 space mission photometry. Based on a Fourier analysis and iterative pre-whitening, we present a classification and evaluate the potential for asteroseismic modelling. We include the lists of pulsation frequencies for three new β Cep pulsators, CD-28 12286, CD-27 10876, LS 3978, and additional pulsation mode frequencies for the known β Cep pulsator HD 164741. In addition, we characterize the regular frequency spacing found in the new pulsator HD 169173, and discuss its origin. We place the newly discovered variables in a colour-magnitude diagram using parallaxes from GaiaDR2 (second data release), showcasing their approximate location in the massive star domain. The identified frequency lists of these multiperiodic pulsators are a good starting point for future forward seismic modelling, after identification of at least one pulsation frequency from high-resolution time-series spectroscopy and/or multicolour photometry.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): asteroseismology - techniques: photometry - stars: individual: (CD-28 12286, CD-27 10876, LS 3978, HD 164741, HD 169173) - stars: massive

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 18

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Number of rows : 18
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 HD 43317 Pu* 06 15 47.0134228488 +04 17 01.095049500 5.82 6.456 6.614     B3IV 114 0
2 HD 256035 * 06 22 58.2414314040 +22 51 46.158064380 9.24 9.63 9.21     O9V:p 34 0
3 HD 46149 Y*O 06 31 52.5319291296 +05 01 59.178678024 7.03 7.80 7.61 7.54 7.36 O8.5V 277 0
4 HD 46202 bC* 06 32 10.4706981304 +04 57 59.764912343 7.60 8.332 8.269 7.98 7.86 O9.2V 285 0
5 HD 49330 bC* 06 47 57.2679459720 +00 46 34.035384504 8.45 9.14 8.95     Bnn(e) 89 0
6 CD-27 10876 * 16 16 15.0462297168 -27 51 19.904137056   11.07 10.95     OB- 6 0
7 CD-28 12286 * 16 41 01.9750176552 -28 43 20.848391256   10.55 10.32     OB- 8 0
8 LS 3978 Pu* 17 13 01.2984241512 -24 12 19.179554040 12.32 12.78 12.41 12.50   B2III 10 0
9 HD 156491 Em* 17 18 38.7684569088 -21 35 21.798721428   9.94 9.54     B3III 9 0
10 HD 157548 * 17 24 51.6296241480 -23 55 33.957398892   9.10 8.80     B5III 8 0
11 HD 164741 bC* 18 03 44.0813322000 -25 18 45.077553432 8.74 9.48 9.19 9.57   B1III 49 0
12 HD 169173 bC* 18 24 08.1576324000 -17 51 48.794845356   10.12 9.93 9.82 9.506 B3Ib 14 0
13 HD 170580 ** 18 30 05.1198164760 +04 03 55.271232360 6.29 6.80 6.69     B2V 102 0
14 HD 180642 bC* 19 17 14.8038514896 +01 03 33.904495728 7.83 8.47 8.29     B1.5II-III 102 0
15 HD 181231 Be* 19 19 42.3695906832 -00 02 59.483615784   8.79 8.58     B5III 31 0
16 BD+43 3310 Pu* 19 37 29.7688619736 +43 24 57.369736800   10.32 10.28     B9IV 52 0
17 HD 186567 Ro* 19 42 48.8430567072 +50 21 39.806399160   9.07 9.21   9.191 F 28 0
18 * 12 Lac bC* 22 41 28.6495065456 +40 13 31.609736580 4.24 5.080 5.229     B2III 357 0

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